Pisces II (dwarf galaxy)
| Pisces II Dwarf Galaxy | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Pisces |
| Right ascension | 22h 58m 31s[1] |
| Declination | +05° 57′ 09″[1] |
| Distance | 585 kly (180 kpc)[1] |
| Type | dSph |
| Apparent dimensions (V) | 2.2+0.2 −0.2′[1] |
| Apparent magnitude (V) | 16.3[1] |
| Other designations | |
| Pisces II | |
Pisces II is a dwarf spheroidal galaxy situated in the Pisces constellation and discovered in 2010 in the data obtained by the Sloan Digital Sky Survey.[1] The galaxy is located at the distance of about 180 kpc from the Sun. It is classified as a dwarf spheroidal galaxy (dSph) meaning that it has an elongated shape with the half-light radius of about 60 pc and ratio of the axis of about 5:3.[1]
Pisces II is one of the smallest and faintest satellites of the Milky Way—its integrated luminosity is about 10,000 times that of the Sun (absolute magnitude of about −5), which corresponds to the luminosity of an average globular cluster. The stellar population of Pisces II consists mainly of moderately old stars formed 10–12 billion years ago. The metallicity of these old stars is low at −2.3 < [Fe/H] < −1.7, which means that they contain at least 80 times less heavy elements than the Sun.[1]
References
| Location |
Milky Way → Milky Way subgroup → Local Group → Virgo Supercluster → Laniakea Supercluster → Observable universe → Universe
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